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Fig. B.1

image

H + K-band spectra of the objects. For each galaxy, we show a central spectrum (black line/lower spectrum) that is extracted from an aperture with diameter corresponding to the FWHM of the seeing (see Table 1). In addition, we show an off-central spectrum (grey line/upper spectrum), centred 1.5 ×FWHM left and right from the nucleus. The spectra are shown in restframe wavelength and have been normalised at 2.159 μm. Important emission and absorption lines have been marked.

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